Crystal structure of propionitrile (CH3CH2CN) determined using synchrotron powder X-ray diffraction
dc.contributor.author | Brand, HEA | en_AU |
dc.contributor.author | Gu, QF | en_AU |
dc.contributor.author | Kimpton, JA | en_AU |
dc.contributor.author | Auchettl, R | en_AU |
dc.contributor.author | Ennis, C | en_AU |
dc.date.accessioned | 2021-11-12T03:37:05Z | en_AU |
dc.date.available | 2021-11-12T03:37:05Z | en_AU |
dc.date.issued | 2020-01 | en_AU |
dc.date.statistics | 2021-11-02 | en_AU |
dc.description.abstract | The structure and thermal expansion of the astronomical molecule propionitrile have been determined from 100 to 150 K using synchrotron powder X-ray diffraction. This temperature range correlates with the conditions of Titan's lower stratosphere, and near surface, where propionitrile is thought to accumulate and condense into pure and mixed-nitrile phases. Propionitrile was determined to crystallize in space group, Pnma (No. 62), with unit cell a = 7.56183 (16) Å, b = 6.59134 (14) Å, c = 7.23629 (14), volume = 360.675 (13) Å3 at 100 K. The thermal expansion was found to be highly anisotropic with an eightfold increase in expansion between the c and b axes. These data will prove crucial in the computational modelling of propionitrile–ice systems in outer Solar System environments, allowing us to simulate and assign vibrational peaks in the infrared spectra for future use in planetary astronomy. © 2020 International Union of Crystallography | en_AU |
dc.description.sponsorship | This work was carried out on the powder diffraction beamline at the Australian Synchrotron; supported by Australian Research Council via the Discover Early Career Research Award (DE150100301). RA was supported by an Australian Government Research Training Program (RTP) Scholarship. RA also thanks the Australian Institute of Nuclear Science and Engineering (AINSE) for their financial support under the AINSE Postgraduate Research Award (PGRA) scheme to enable this work | en_AU |
dc.identifier.citation | Brand, H. E. A, Gu, Q., Kimpton, J. A., Auchettl, R.& Ennis, C.(2020). Crystal structure of propionitrile (CH3CH2CN) determined using synchrotron powder X-ray diffraction. Journal of Synchrotron Radiation, 27, 212-216. doi:10.1107/S1600577519015911 | en_AU |
dc.identifier.issn | 1600-5775 | en_AU |
dc.identifier.journaltitle | Journal of Synchrotron Radiation | en_AU |
dc.identifier.pagination | 212-216 | en_AU |
dc.identifier.uri | https://doi.org/10.1107/S1600577519015911 | en_AU |
dc.identifier.uri | https://apo.ansto.gov.au/dspace/handle/10238/12234 | en_AU |
dc.identifier.volume | 27 | en_AU |
dc.language.iso | en | en_AU |
dc.publisher | International Union of Crystallography | en_AU |
dc.subject | Crystal structure | en_AU |
dc.subject | Synchrotrons | en_AU |
dc.subject | X-ray diffraction | en_AU |
dc.subject | Thermal expansion | en_AU |
dc.subject | Ice | en_AU |
dc.subject | Planetary atmospheres | en_AU |
dc.subject | Satellites | en_AU |
dc.subject | Nitriles | en_AU |
dc.title | Crystal structure of propionitrile (CH3CH2CN) determined using synchrotron powder X-ray diffraction | en_AU |
dc.type | Journal Article | en_AU |
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